Circular No. 3827 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. TWX 710-320-6842 ASTROGRAM CAM Telephone 617-864-5758 COMET SUGANO-SAIGUSA-FUJIKAWA (1983e) Observations by E. Barker with the McDonald Observatory's 1.7-m reflector on June 9 showed the comet to have a very weak, but essentially stellar condensation of mag 18-19. Emissions of CN, C2 and C3 were detected, but there was little or no continuum. SUPERNOVA IN NGC 4699 J. Maza, University of Chile, telexes that M. Wischnjewsky has discovered a supernova in NGC 4699 on plates taken by L. E. Gonzalez at Cerro El Roble. The object brightened from mpg 17 on June 6.12 UT to mpg 14 on June 10.12. The supernova, 148" east and 131" north of the galaxy's nucleus, is located at the position R.A. = 12h46m36s41, Decl. = -8deg21'21".9 (equinox 1950.0). BL TELESCOPII I. Ferrin, Universidad de Los Andes, Merida, Venezuela, writes: "According to the ephemeris by Gaposhkin (1970, A.J. 75, 641), the remarkable supergiant eclipsing binary BL Tel (R.A. = 19h02m7, Decl. = -51deg30', equinox 1950.0) is about to enter eclipse. The nominal dates (eclipse begins Aug. 2, ends Oct. 19) are uncertain because of a possible period change in 1950. At maximum V = 7.0. At mid-eclipse (nominally Sept. 10) V = 9.1, but minimum brightness in the past has varied from V = 8.47 to V = 9.29." COMET IRAS (1983f) J. Gibson provides the following precise measurement for the third observation reported on IAUC 3818: 1983 UT R.A. (1950.0) Decl. May 31.17714 9 16 45.91 - 8 06 30.6 PERIODIC COMET TEMPEL 1 (1982j) Further total visual magnitude estimates: May 12.14, 9.8 (J. Bortle, Stormville, NY, 0.32-m reflector; tail in p.a. 220); 14.98, 10.3 (J. D. Shanklin, Cambridge, Eng., 20 x 80 binoculars); 17.87, 9.9 (J.-C. Merlin, Le Creusot, France, 0.26-m reflector); 29.86, 9.6 (Merlin); June 4.94, 9.3 (Merlin); 10.93, 9.4 (Merlin). 1983 June 13 (3827) Brian G. Marsden
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